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History of Astronomy

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Title: History of Astronomy


1
History of Astronomy
  • The knowledge of the Ancients

2
Passage of astronomical knowledge
Ancient Babylon
Ancient Egypt
Ancient Greece
Ancient Roman Empire
3
Mesopotamia/Babylon
Modern political boundaries
Ancient Babylon
4
Mesopotamia/Babylon
5
Ancient Egypt
Nile River Valley
Great Pyramid of Kufu
6
Ancient Greece
7
Ancient Greece
8
Ancient Rome
9
(No Transcript)
10
Greek Astronomy
11
Greek Astronomy
  • About 624 BC to 547 BC
  • One of the earliest Greek philosophers.
  • His areas of interest included geometry and
    astronomy.
  • There are no books or writings that have survived
    from Thales.

Thales
12
Greek Astronomy
  • About 569 BC to 475 BC
  • One of the greatest mathematicians of all time.
  • Founded secret society based on his mathematical
    discoveries and their religious implications.
  • Since the society was extremely secretive, very
    little is known about his life or personal works.

Pythagoras
13
Greek Astronomy
  • 427 BC to 347 BC
  • Well known for political and social philosophy
    but he also made contributions to astronomy.
  • He was most noted for his belief in the perfect
    and unchanging nature of the heavens.
  • Plato was the head of the School of Athens was
    Aristotles teacher.

Plato
14
Greek Astronomy
Aristotle
  • 384 BC to 322 BC
  • Founded his own school called the Lyceum in
    Athens
  • Made contributions to all areas of philosophy but
    math was his weakness
  • He did not believe that empirical evidence was
    necessary to prove ideas.

15
Greek Astronomy
Aristotle
  • Aristotle is one the first to attempt to create a
    scientific model of the universe.
  • This model has now become known as the
    Geocentric Model which places the imperfect
    Earth at the center and all of the perfect
    celestial objects go around us in perfect
    circular motion

16
Greek Astronomy
Euclid
  • About 325 BC to 265 BC
  • Great mathematician but so little is known about
    him that people question whether he was an actual
    person or a group of mathematicians.

17
Greek Astronomy
  • The book Elements is possible the most famous
    and long lasting math text books in history.

Euclid
18
Greek Astronomy
Aristarchus
  • About 310 BC to 230 BC
  • We have no writings that have survived but
    Aristarchus is referred to in the writings of
    other philosophers

19
Greek Astronomy
Aristarchus
  • Most noted for proposing the idea of a
    heliocentric universe with the earth as one of
    the planets moving around the Sun.
  • Aristarchus is the first to attempt to measure
    the relative distance between the Earth-Moon and
    the Earth-Sun without the aid of trigonometry.
  • Actual angle 89 50 not 87

20
Greek Astronomy
Eratosthenes
  • 276 BC to 194 BC
  • Librarian at the Great Library of Alexandria in
    Egypt.
  • Developed a calendar with a leap year.
  • Measured the circumference of the Earth in 325 BC
    !!
  • Achieved an accuracy of about 90 of the actual
    number.

21
Greek Astronomy
  • 190 BC to 120 BC
  • Hipparchus is consider the first great astronomer
    and scientist
  • Hipparchus is one of the first of the ancient
    philosophers to realize that ideas must be proven
    with empirical evidence.
  • He realized that more data meant more certainty
    in the idea or model

Hipparchus
22
Greek Astronomy
Hipparchus
  • Created highly accurate star atlases in an
    attempt to measure the length of the year more
    accurately.
  • He measured the length of the year to within 6.5
    minutes of the actual time.
  • He discovered precession by examining ancient
    star position data (mostly Mesopotamian) and
    comparing them to his own measurements.

23
Greek Astronomy
Hipparchus
  • Based on measurements during an eclipse, he is
    able to place a range on the distance to the
    moon.
  • He estimated it to be between 59 and 67 Earth
    diameters. The actual number is 60.
  • He marks the first truly scientific astronomical
    mind and his influence is still felt today.

24
Greek Astronomy
  • About 85 AD to 165 AD
  • Ptolemy is the most influential astronomer in his
    day and his models of the universe will prevail
    for the next 1400 years
  • He is a great admirer of Hipparchus and his
    rigorous method of verifying ideas with empirical
    data.
  • Ptolemy is also accused of stealing ideas without
    crediting his source.

Ptolemy
25
Greek Astronomy
  • Ptolemy is a great proponent of the geocentric
    model.
  • He saw that there were problems with Aristotles
    simplistic idea of a geocentric model.
  • Ptolemy employed an old idea of epicycles to
    explain help explain the discrepancies in the
    evidence for geocentrism.
  • Although he was able to make more accurate
    predictions than previous astronomers, his model
    still failed to be completely accurate.

Ptolemy
26
Ancient Greece
27
Ancient Rome
The Romans most important contribution to the
field of astronomy is the enforcement of a
systematic calendar that would account for fact
that the year is about ¼ of a day more 365 days.
The astronomers of Julius Caesar convinced him to
create the Julian Calendar which adds one day to
the calendar every 4 years to account for the
time we had skipped. This is known as a leap
year.
28
Geocentric or Heliocentric?
  • Of the early philosophers, only Hipparchus
    favored the heliocentric model
  • Most philosophers thought that the evidence
    supported the Geo model more than the Helio model
  • What was the evidence? Lets Look.

29
Geocentric Evidence
  • Everything appears to revolve around the Earth
    each day (diurnal motion).
  • There is no observable parallax of the stars,
    planets, Moon, or Sun.
  • The motions of the stars and heavens are perfect
    circles.
  • The heavens were unchanging but the Earth was not.

30
Problems With the Geocentric Model
  • The planets appear to change brightness, implying
    a change of distance.
  • The planets undergo retrograde motion (they move
    backwards compared to the direction the Sun
    moves).
  • The Sun, Moon, and Planets do not move at the
    same speed all the time.
  • Mercury and Venus are never seen at opposition
    (they always appear close to the Sun.

31
Evidence of the Heliocentric Model
  • The changing brightness of the planets is
    explained by the Earth getting closer and farther
    from the planets during our orbit of the Sun.
  • Our passing planets explain the retrograde motion
    of the outer planets.
  • Mercury and Venus are not seen at opposition
    because they orbit the sun, just as we do.

32
Problems with the Heliocentric Model
  • The changing speeds of the Sun, Moon, and planets
    is not explained by simply placing the Sun at the
    center of the universe.
  • We do not feel the Earth moving or the atmosphere
    being pulled away as we fly around the Sun.
  • If the Earth were spinning, wouldnt we be thrown
    off into space?
  • Why is there no parallax due to our spin or our
    orbit?

33
So Which is Right?
  • The ancients favored the geocentric model because
    it seemed impossible to believe that the Earth
    was moving.
  • During ancients times, the mathematical and
    scientific tools were not available to answer the
    question without dispute.
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